Published April 1989
| Version v1
Journal article
A rotating Bianchi type II cosmological model with viscous fluid and heat flux
Creators
- 1. Gujarat Univ., Ahmedabad (India). Dept. of Mathematics
- 2. Ohio State Univ., Columbus (USA). Dept. of Mathematics
Description
An exact solution of Einstein field equations corresponding to viscous fluid and heat flux is derived. The solution describes a rotating spatially homogeneous Bianchi II universe containing viscous fluid and heat flow. In the model, the shear scalar and the expansion scalar are linearly related. Also a linear relation between the shear viscosity coefficient and the scalar of expansion is assumed. Some physical and kinematical features of the model have been explored. Some interesting particular cases are also discussed. (author). 12 refs
Additional details
Publishing Information
- Journal Title
- Journal of Mathematical and Physical Sciences
- Journal Volume
- 23
- Journal Issue
- 2
- Series
- J. Math. Phys. Sci.
- Journal Page Range
- 135-146
- ISSN
- 0047-2557
- CODEN
- JMPSB
INIS
- Country of Publication
- India
- Country of Input or Organization
- India
- INIS RN
- 20082184
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL MODELS; EINSTEIN FIELD EQUATIONS; HEAT FLUX; ROTATION; SCALARS; UNIVERSE; VISCOSITY
- Descriptors DEC
- EQUATIONS; FIELD EQUATIONS; MATHEMATICAL MODELS